Study of CR primaries and their cascades at E0 = 10-100 TeV through EAS-TOP and MACRO
| dc.creator | EAS-TOP, The | |
| dc.creator | Collaborations, MACRO | |
| dc.date | 2001-12-20 | |
| dc.date.accessioned | 2026-07-25T18:32:28Z | |
| dc.description | A measurement of the lateral distribution of Cherenkov light in Extensive Air Showers (EAS) at E0 = 10-100 TeV and a study of the compatibility of the photon number spectra with the expectations from the direct measurements of p and He spectra and the Corsika-QGSJET propagation code in the atmosphere have been performed at the National Gran Sasso Laboratories by the EAS-TOP and MACRO arrays. The telescope array of EAS-TOP has been used as the Cherenkov light detector. The muon tracking system of MACRO in the deep underground Gran Sasso Laboratories (Emuon> 1.3 TeV) served as the EAS detector, including core localization and arrival direction. | |
| dc.description | Contribution to TAUP2001, Sep. 8-12, 2001, Assergi (Italy) | |
| dc.identifier | https://arxiv.org/abs/astro-ph/0112475 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/0112475 | |
| dc.identifier.uri | https://dspace.dare.co.zw/handle/123456789/56140 | |
| dc.subject | Astrophysics | |
| dc.title | Study of CR primaries and their cascades at E0 = 10-100 TeV through EAS-TOP and MACRO | |
| dc.type | text |